PIRSA:11110002

Quasi-single and Multiple Field Inflation

APA

(2011). Quasi-single and Multiple Field Inflation. Perimeter Institute. https://pirsa.org/11110002

MLA

Quasi-single and Multiple Field Inflation. Perimeter Institute, Nov. 08, 2011, https://pirsa.org/11110002

BibTex

          @misc{ pirsa_PIRSA:11110002,
            doi = {10.48660/11110002},
            url = {https://pirsa.org/11110002},
            author = {},
            keywords = {Cosmology},
            language = {en},
            title = {Quasi-single and Multiple Field Inflation},
            publisher = {Perimeter Institute},
            year = {2011},
            month = {nov},
            note = {PIRSA:11110002 see, \url{https://pirsa.org}}
          }
          

Abstract

The talk consists of two parts: (1) Quasi-single inflation, where the isocurvature direction has mass of order Hubble parameter. This part is based on 0911.3380 and new results about higher mass, and a sharp turn in trajectory. (2) Multi-stream inflation, where the inflationary trajectory bifurcates. This part is based on 0903.2123, 1006.5021 and a on-going project on calculating the bifurcation probability in a complicated landscape.